High Energy Neutrinos: Sources and Fluxes
arXiv:astro-ph/0511641 · doi:10.1088/1742-6596/39/1/103
Abstract
We discuss briefly the potential sources of high energy astrophysical neutrinos and show estimates of the neutrino fluxes that they can produce. A special attention is paid to the connection between the highest energy cosmic rays and astrophysical neutrinos.
arXiv comment7 pages, 2 figures, submitted to the Proceedings of TAUP 2005 workshop, corrected left panel of figure 2
References in corpus (24)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs
- High Energy Neutrinos from Astrophysical Sources: An Upper Bound
- COSMOLOGICAL GAMMA RAY BURSTS AND THE HIGHEST ENERGY COSMIC RAYS
- BL Lac Objects in the Synchrotron Proton Blazar Model
- High-energy particle acceleration in the shell of a supernova remnant
- Neutrinos from propagation of ultra-high energy protons
- Very high energy gamma rays from the direction of Sagittarius A*
- Monte-Carlo simulations of photohadronic processes in astrophysics
- Calibration of cameras of the H.E.S.S. detector
- On the cosmic ray bound for models of extragalactic neutrino production
- Photohadronic Neutrinos from Transients in Astrophysical Sources
- TeV Neutrinos from Successful and Choked Gamma-Ray Bursts
- High Energy Neutrinos from Gamma Ray Bursts
- Gamma-ray production in supernova remnants
- Implications of Particle Acceleration in Active Galactic Nuclei for Cosmic Rays and High Energy Neutrino Astronomy
- Ultra-High Energy Neutrino Fluxes: New Constraints and Implications
- Cosmogenic Neutrinos from Ultra-High Energy Nuclei
- Empirical Constraints on Source Properties and Host Galaxies of Cosmological Gamma-Ray Bursts
- Neutrinos: the Key to UHE Cosmic Rays
- Gamma Rays and Neutrinos from a Powerful Cosmic Accelerator
- High Energy Neutrinos from Gamma Ray Bursts: Event Rates in Neutrino Telescopes
- High energy neutrinos from a slow jet model of core collapse supernovae
- Neutrino Event Rates from Gamma Ray Bursts